Phes ch22


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Earth Science Origin of Modern Astronomy

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  • Who is Stan Hatfield and Ken Pinzke
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  • Phes ch22

    1. 1. Prentice Hall EARTH SCIENCE Tarbuck Lutgens 
    2. 2. Chapter 22 Origin of Modern Astronomy
    3. 4. Objectives (22.1): <ul><li>Describe the science and study of astrology, as opposed to astronomy </li></ul><ul><li>Identify the accomplishments of early astronomers. </li></ul>
    4. 5. 22.1 Early Astronomy  Astronomy is the science that studies the universe. It includes the observation and interpretation of celestial bodies and phenomena.  The Greeks used philosophical arguments to explain natural phenomena.  The Greeks also used some observational data. Ancient Greeks
    5. 6. Astrolabe
    6. 7. Calculating Earth’s Circumference
    7. 8. 22.1 Early Astronomy  Geocentric Model • In the ancient Greeks’ geocentric model, the moon, sun, and the known planets—Mercury, Venus, Mars, and Jupiter—orbit Earth.  Heliocentric Model • In the heliocentric model, Earth and the other planets orbit the sun. Ancient Greeks
    8. 9. Geocentric and Heliocentric Models
    9. 10. 22.1 Early Astronomy  Ptolemaic System • Ptolemy created a model of the universe that accounted for the movement of the planets. • Retrograde motion is the apparent westward motion of the planets with respect to the stars. Ancient Greeks
    10. 11. Doppler Effect and Retrograde Motion <ul><li>As the viewer MOVES, what is observed appears/sounds different. </li></ul><ul><li>This is the same principle as RETROGRADE MOTION. As we look at a planet, the planet and the earth are both moving. </li></ul>
    11. 12. Youtube examples <ul><li>On side of road viewing Motorcycle: http:// = qWKqdevDuss&feature =related </li></ul><ul><li>Train illustration with sound waves: </li></ul><ul><li>http:// =iN3fO5l4Rww </li></ul><ul><li>On Earth viewing Mars: http:// =72FrZz_zJFU </li></ul>
    12. 13. Retrograde Motion
    13. 14. 22.1 Early Astronomy  Nicolaus Copernicus • Copernicus concluded that Earth is a planet. He proposed a model of the solar system with the sun at the center . The Birth of Modern Astronomy
    14. 15. 22.1 Early Astronomy  Johannes Kepler • Kepler discovered three laws of planetary motion: 1. Orbits of the planets are elliptical. 2. Planets revolve around the sun at varying speed. 3. There is a proportional relationship between a planet’s orbital period and its distance to the sun. The Birth of Modern Astronomy
    15. 16. 22.1 Early Astronomy  Johannes Kepler • An ellipse is an oval-shaped path . • An astronomical unit (AU) is the average distance between Earth and the sun; it is about 150 million kilometers . The Birth of Modern Astronomy
    16. 17. Planet Revolution
    17. 18. 22.1 Early Astronomy  Galileo Galilei • Galileo’s most important contributions were his descriptions of the behavior of moving objects. • He developed his own telescope and made important discoveries: 1. Four satellites, or moons, orbit Jupiter. 2. Planets are circular disks, not just points of light. 3. Venus has phases just like the moon. 4. The moon’s surface is not smooth. 5. The sun has sunspots, or dark regions.
    18. 19. The Solar System Model Evolves
    19. 20. 22.1 Early Astronomy  Sir Isaac Newton • Although others had theorized the existence of gravitational force, Newton was the first to formulate and test the law of universal gravitation.  Universal Gravitation (Gravity) • Gravitational force decreases with distance. • The greater the mass of an object, the greater is its gravitational force.
    20. 21. Gravity’s Influence on Orbits
    21. 22. Ch. 22.2 Objectives <ul><li>The Earth-Moon-Sun System. </li></ul><ul><li>Describe the movements of the Earth known as rotation, revolution, and precession. </li></ul><ul><li>Explain why eclipses are relatively rare events. </li></ul>
    22. 23. 22.2 The Earth–Moon–Sun System  The two main motions of Earth are rotation and revolution. Precession is a third and very slow motion of Earth’s axis. Motions of Earth
    23. 24. 22.2 The Earth–Moon–Sun System  Rotation • Rotation is the turning, or spinning, of a body on its axis. • Two measurements for rotation: 1. Mean solar day is the time interval from one noon to the next, about 24 hours. 2. Sidereal day is the time it takes for Earth to make one complete rotation (360º) with respect to a star other than the sun—23 hours, 56 minutes, 4 seconds. Motions of Earth
    24. 25. 22.2 The Earth–Moon–Sun System  Revolution • Revolution is the motion of a body, such as a planet or moon, along a path around some point in space. • Perihelion is the time in January when Earth is closest to the sun. • Aphelion is the time in July when Earth is farthest from the sun. Motions of Earth
    25. 26. 22.2 The Earth–Moon–Sun System  Earth’s Axis and Seasons • Because of the inclination of Earth’s axis to the plane of the ecliptic, Earth has its yearly cycle of seasons. (23.5 Degrees) • The plane of the ecliptic is an imaginary plane that connects Earth’s orbit with the celestial sphere. Motions of Earth
    26. 27. 22.2 The Earth–Moon–Sun System  Precession • Precession traces out a cone over a period of 26,000 years.  Earth–Sun Motion • The solar system speeds in the direction of the star Vega. • The sun revolves around the galaxy. • Earth is presently approaching one of its nearest galactic neighbors, the Great Galaxy in Andromeda. Motions of Earth
    27. 28. Precession
    28. 29. 22.2 The Earth–Moon–Sun System  Perigee is the point at which the moon is closest to Earth.  Apogee is the point at which the moon is farthest from Earth. Motions of the Earth–Moon System
    29. 30. 22.2 The Earth–Moon–Sun System  Phases of the Moon • The phases of the moon are the progression of changes in the moon’s appearance during the month. • Lunar phases are a result of the motion of the moon and the sunlight that is reflected from its surface. Motions of the Earth–Moon System
    30. 31. Phases of the Moon
    31. 32. Phases of the Moon <ul><li>http:// = nXseTWTZlks </li></ul>
    32. 33. Lunar Motions
    33. 34. 22.2 The Earth–Moon–Sun System  Solar eclipses occur when the moon moves in a line directly between Earth and the sun, casting a shadow on Earth.  During a new-moon or full-moon phase, the moon’s orbit must cross the plane of the ecliptic for an eclipse to take place.  Lunar eclipses occur when the moon passes through Earth’s shadow. Eclipses
    34. 35. Solar Eclipse
    35. 36. Lunar Eclipse
    36. 37. Eclipses: Solar and Lunar <ul><li>http:// =dqreLkR0MoM </li></ul>
    37. 38. Ch. 22.3 <ul><li>Objectives:  The Earth’s Moon </li></ul><ul><li>Describe the physical features  of the lunar surface and how they were formed. </li></ul><ul><li>Explain the history of the moon. </li></ul><ul><li>Starter: </li></ul><ul><li>Describe the three motions of the Earth, draw them. </li></ul><ul><li>What phase of the moon are we in now?  Draw a picture.  How is this information used by different cultures? </li></ul>
    38. 39. 22.3 Earth’s Moon • A crater is the depression at the summit of a volcano or a depression produced by a meteorite impact.  Craters • Most craters were produced by the impact of rapidly moving debris. • Rays are any of a system of bright, elongated streaks, sometimes associated with a crater on the moon. The Lunar Surface
    39. 40. The Moon’s Surface Mare Tranquillitatus (Sea of Tranquility ) Mare Imbrium (Sea of Rains ) Kepler Crater Copernicus Crater
    40. 41. Formation of a Crater
    41. 42. 22.3 Earth’s Moon • Most of the lunar surface is made up of densely pitted, light-colored areas known as highlands.  Highlands • Maria , ancient beds of basaltic lava, originated when asteroids punctured the lunar surface, letting magma bleed out.  Maria • A rille is a long channel associated with lunar maria. A rille looks similar to a valley or a trench. The Lunar Surface
    42. 43. 22.3 Earth’s Moon • The lunar regolith is a thin, gray layer on the surface of the moon, consisting of loosely compacted, fragmented material believed to have been formed by repeated impacts of meteorites.  Regolith The Lunar Surface
    43. 44. Major Topographic Features of the Moon
    44. 45. 22.3 Earth’s Moon  The most widely accepted model for the origin of the moon is that when the solar system was forming, a body the size of Mars impacted Earth. The resulting debris was ejected into space, began orbiting around Earth, and eventually united to form the moon. Lunar History
    45. 46. Video: The Moon <ul><li>http:// =m8P5ujNwEwM&feature= player_embedded#at =560 </li></ul>
    46. 47. Quiz Topics <ul><li>Quiz: </li></ul><ul><li>Heliocentric </li></ul><ul><li>Geocentric </li></ul><ul><li>Newton </li></ul><ul><li>Galileo </li></ul><ul><li>Copernicus </li></ul><ul><li>Motions of Earth </li></ul><ul><li>Geography of the Moon </li></ul>
    47. 48. Formation of Earth’s Moon